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V: 0
V: 0

... The student is expected to explore how different wavelengths of the electromagnetic spectrum such as light and radio waves are used to gain information about distances and properties of components in the universe. ...
33-3 - Fremont Peak Observatory
33-3 - Fremont Peak Observatory

... only 700 light-years from Earth! There are no really bright stars close to the Helix. When I first viewed this object a few years back, I had to get in the general neighborhood with my eyepiece, and my mount’s clutch pins loose. I scanned the area until I saw a faint, hazy cloud which contrasts to t ...
Astronomical Distance Determination • etc.
Astronomical Distance Determination • etc.

... Globular clusters must orbit around the center of mass of the galaxy! Thus, assuming the clusters are distributed uniformly around the galaxy, he measured the 3D distribution of clusters (using Cepheid variables) and then assumed that the center of that distribution was where the center of the galax ...
Antares - Emmi
Antares - Emmi

... Antares is in the constellation scorpio The Scorpio constellations story is an ancient Greek myth. Orion the hunter was the best hunter in the world and the most handsome man. He bragged that he would kill every animal on Earth. Apollo guardian of the cows pleaded with Hera the queen of the gods t ...
Pulsating Variable Stars and The Hertzsprung - Chandra X
Pulsating Variable Stars and The Hertzsprung - Chandra X

The Lyre of Orpheus - InteractiveStars.com
The Lyre of Orpheus - InteractiveStars.com

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Surveying the Stars

... • Just about anything you want to find out about a star, you can find out if it’s in an eclipsing binary system (well, maybe a slight exaggeration, but not much) ...
Review: How does a star`s mass determine its life story?
Review: How does a star`s mass determine its life story?

... White dwarf supernova: A white dwarf in close binary system reaches the white dwarf mass limit, causing an explosion. Carbon fusion may re-ignite for a brief time for the explosion. The Energy released is enough to destroy the star completely, an there is NO neutron star left behind. ...
Name Date Life and Death of a Star 2015 1. In the main
Name Date Life and Death of a Star 2015 1. In the main

... B. collision with another star C. gravitational collapse of the core of a massive star 29. When helium fusion takes over in a star's core, what happens? A. the energy output decreases B. energy output stays the same C. the energy output increases 30. A star that is gravitationally bound to another m ...
distant stars nearby star parallax angle The principle of geometrical
distant stars nearby star parallax angle The principle of geometrical

... didn’t know the distances to these stars, we wouldn’t know that Betelgeuse is a red giant star, with a much greater intrinsic brightness than Vega (and much larger diameter). Nor would we know that many stars visible in the night sky are much like the Sun, but just much, much farther away so they ap ...
Not Always the Southern Cross! Which Way`s South?
Not Always the Southern Cross! Which Way`s South?

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Diapositiva 1

... Side View of the Milky Way The “halo” is really the “stellar halo” – turns out there’s actually a larger halo we can’t even see! ...
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View the presentation slides

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Oct 06, 2001

... C. It is moving away from the Earth. D. It will live longer than a B spectral class main sequence star. E. It is the same size as a red giant star of the same temperature. 28. There are reported to be about 6,000 stars visible to the naked eye. How many of those stars would you expect to be part of ...
mslien~1
mslien~1

... From above the Jeans criterion can be derived as M c  M J where the Jeans mass MJ is given by the RHS of ...
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E3 – Stellar distances

... • At distances greater than Mpc, neither parallax nor spectroscopic parallax can be relied upon to measure the distance to a star. • When we observe another galaxy, all of the stars in that galaxy are approximately the same distance away from the earth. What we really need is a light source of known ...
A0620-00 poster
A0620-00 poster

... As the brightest dwarf nova and one of the brightest cataclysmic variables of any kind, SS Cygni has been extensively observed. Its outbursts, for example, have been continuously monitored since 1896 and their properties are the gold standard against which accretion disk instability models for dwarf ...
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A105 Stars and Galaxies

... hydrogen into helium in their cores •Massive main-sequence stars are hot (blue) and luminous •Less massive stars are cooler (yellow or red) and fainter ...
Stars and Galaxies
Stars and Galaxies

... • Mass of massive stars 6x that of sun • Take same path as medium-sized stars except for after red giant stage they do not become white dwarfs • Carbon atoms continue to fuse creating heavier elements like oxygen & nitrogen • Core of massive star so hot that fusion continues until the heavy element ...
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Sources of Gravitational Waves Peter Shawhan

... Orbit will continue to decay (inspiral) over the next ~300 million years, until… ...
Distance measurement in Astronomy
Distance measurement in Astronomy

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The Rigel Star - Emmi

... angry about the death of her companion, but forgave Apollo when he helped her hang his image in the sky so that he wouldn’t be forgotten. The Greeks said that this is why the constellation of Orion is visible in the winter, but wavers and vanishes when Scorpio appears in the summer. ...
OUR UNIVERSE Problem Set 7 Solutions Question A1 Question A2
OUR UNIVERSE Problem Set 7 Solutions Question A1 Question A2

... (a) The hydrogen-burning main sequence phase, As the proto-star collapses under its own gravity its atoms (hydrogen about 70 % and helium about 25 %) heat up because they exchange gravitational potential energy for kinetic energy, eventually the atoms in the core reach temperatures of about 15 milli ...
Milky Way thin disk
Milky Way thin disk

Winter 2014
Winter 2014

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Lyra



Lyra (/ˈlaɪərə/; Latin for lyre, from Greek λύρα) is a small constellation. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, and hence sometimes referred to as Aquila Cadens or Vultur Cadens. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus. Lyra is visible from the northern hemisphere from spring through autumn, and nearly overhead, in temperate latitudes, during the summer months. From the southern hemisphere, it is visible low in the northern sky during the winter months.The lucida or brightest star—and one of the brightest stars in the sky—is the white main sequence star Vega, a corner of the Summer Triangle. Beta Lyrae is the prototype of a class of stars known as Beta Lyrae variables, binary stars so close to each other that they become egg-shaped and material flows from one to the other. Epsilon Lyrae, known informally as the Double Double, is a complex multiple star system. Lyra also hosts the Ring Nebula, the second-discovered and best-known planetary nebula.
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